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The Geological Society offers grades of membership for every stage of your career, from student to retirement. Find out about the benefits of membership, and how we can help you achieve and maintain Chartered status.

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Geoscientist is the Fellowship magazine of the Geological Society: with news about science, people, the Society, features, reviews, opinion, letters and forthcoming events. All this, and more, can be found sooner here, in our online version.

The Geological Society of London is the UK national society for geoscience, providing support to over 11,500 members in the UK and overseas. Founded in 1807, we are the oldest geological society in the world.

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Books have damaged covers (on spine, corners and edges) - interior pages are all OK. Regular prices:
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Fellow's price: £50.00
Other societies price: £60.00Please see SP412 for regular stock.The Himalayan mountain belt, which developed during the India–Asia collision starting about 55 Ma ago, is a dramatically active orogen and it is regarded as the classic collisional orogen. It is characterized by an impressively continuous 2500 km of tectonic units, thrusts and normal faults, as well as large volumes of high-grade metamorphic rocks and granites exposed at the surface. This constitutes an invaluable field laboratory, where amazing crustal sections can be observed directly in very deep gorges. It is possible to unravel the tectonic and metamorphic evolution of litho-units, to observe the mechanisms of exhumation of deep-seated rocks and the propagation of the deformation. Himalayan tectonics has been the target of many studies from numerous international researchers over the years. In the last 15 years there has been an explosion of data and theories from both geological and geophysical perspectives.

This book presents the results of integrated multidisciplinary studies, including geology, petrology, magmatism, geochemistry, geochronology and geophysics, of the structures and processes affecting the continental lithosphere. These processes and their spatial and temporal evolution have major consequences on the geometry and kinematics of the India–Eurasia collision zone.

Published online 18/08/2015. Print copies available from 22/09/2015.

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